Advanced Virgo is the successor of the initial Virgo gravitational wave detector. This new interferometer will use the infrastructure of its predecessor but aims to be 10 times more sensitive. This presentation will give an overview of the Advanced Virgo design and the technical choices behind it. The different subsystem will be detailed as well as the challenges that can be expected. Finally the up-to-date installation progress and expected schedule will be given.

Advanced Virgo Status / Degallaix, J; Accadia, T; Acernese, F; Agathos, M; Allocca, A; Astone, P; Ballardin, G; Barone, F; Barsuglia, M; Basti, A; Bauer, Ts; Bebronne, M; Bejger, M; Beker, Mg; Bitossi, M; Bizouard, Ma; Blom, M; Bondu, F; Bonelli, L; Bonnand, R; Boschi, V; Bosi, L; Bouhou, B; Bradaschia, C; Branchesi, M; Briant, T; Brillet, A; Brisson, V; Bulik, T; Bulten, Hj; Buskulic, D; Buy, C; Cagnoli, G; Calloni, E; Canuel, B; Carbognani, F; Cavalier, F; Cavalieri, R; Cella, G; Cesarini, E; Chassande-Mottin, E; Chincarini, A; Chiummo, A; Cleva, F; Coccia, E; Cohadon, Pf; Colacino, Cn; Colla, A; Colombini, M; Conte, A; Coulon, Jp; Cuoco, E; D'Antonio, S; Dattilo, V; Davier, M; Day, R; De Rosa, R; Debreczeni, G; Del Pozzo, W; Di Fiore, L; Di Lieto, A; Di Virgilio, A; Dietz, A; Drago, M; Endroczi, G; Fafone, V; Ferrante, I; Ferrini, F; Fidecaro, F; Fiori, I; Flaminio, R; Forte, La; Fournier, Jd; Franc, J; Franco, S; Frasca, S; Frasconi, F; Galimberti, M; Gammaitoni, L; Garufi, F; Gaspar, Me; Gemme, G; Genin, E; Gennai, A; Giazotto, A; Gouaty, R; Granata, M; Guidi, Gm; Heidmann, A; Heitmann, H; Hello, P; Hemming, G; Jaranowski, P; Jonker, Rjg; Kasprzack, M; Kowalska, I; Krolak, A; Leroy, N; Letendre, N; Li, Tgf; Lorenzini, M; Loriette, V; Losurdo, G; Majorana, E; Maksimovic, I; Malvezzi, V; Man, N; Mantovani, M; Marchesoni, F; Marion, F; Marque, J; Martelli, F; Masserot, A; Meidam, J; Michel, C; Milano, L; Minenkov, Y; Mohan, M; Morgado, N; Mosca, S; Mours, B; Naticchioni, L; Neri, I; Nocera, F; Palladino, L; Palomba, C; Paoletti, F; Paoletti, R; Parisi, M; Pasqualetti, A; Passaquieti, R; Passuello, D; Pichot, M; Piergiovanni, F; Pinard, L; Poggiani, R; Prodi, Ga; Punturo, M; Puppo, P; Rabeling, Ds; Racz, I; Rapagnani, P; Re, V; Regimbau, T; Ricci, F; Robinet, F; Rocchi, A; Rolland, L; Romano, R; Rosinska, D; Ruggi, P; Saracco, E; Sassolas, B; Sentenac, D; Sperandio, L; Sturani, R; Swinkels, B; Tacca, M; Taffarello, L; ter Braack, Apm; Toncelli, A; Tonelli, M; Torre, O; Tournefier, E; Travasso, F; Vajente, G; van den Brand, Jfj; Van den Broeck, C; van der Putten, S; Vasuth, M; Vavoulidis, M; Vedovato, G; Verkindt, D; Vetrano, F; Vicere, A; Vinet, Jy; Vitale, S; Vocca, H; Ward, Rl; Was, M; Yvert, M; Zadrozny, A; Zendri, Jp. - 467:(2013). (Intervento presentato al convegno 9TH LISA SYMPOSIUM tenutosi a Paris, FRANCE).

Advanced Virgo Status

Drago, M;Frasca, S;Majorana, E;Rapagnani, P;Ricci, F;
2013

Abstract

Advanced Virgo is the successor of the initial Virgo gravitational wave detector. This new interferometer will use the infrastructure of its predecessor but aims to be 10 times more sensitive. This presentation will give an overview of the Advanced Virgo design and the technical choices behind it. The different subsystem will be detailed as well as the challenges that can be expected. Finally the up-to-date installation progress and expected schedule will be given.
2013
9TH LISA SYMPOSIUM
Status report Virgo+
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
Advanced Virgo Status / Degallaix, J; Accadia, T; Acernese, F; Agathos, M; Allocca, A; Astone, P; Ballardin, G; Barone, F; Barsuglia, M; Basti, A; Bauer, Ts; Bebronne, M; Bejger, M; Beker, Mg; Bitossi, M; Bizouard, Ma; Blom, M; Bondu, F; Bonelli, L; Bonnand, R; Boschi, V; Bosi, L; Bouhou, B; Bradaschia, C; Branchesi, M; Briant, T; Brillet, A; Brisson, V; Bulik, T; Bulten, Hj; Buskulic, D; Buy, C; Cagnoli, G; Calloni, E; Canuel, B; Carbognani, F; Cavalier, F; Cavalieri, R; Cella, G; Cesarini, E; Chassande-Mottin, E; Chincarini, A; Chiummo, A; Cleva, F; Coccia, E; Cohadon, Pf; Colacino, Cn; Colla, A; Colombini, M; Conte, A; Coulon, Jp; Cuoco, E; D'Antonio, S; Dattilo, V; Davier, M; Day, R; De Rosa, R; Debreczeni, G; Del Pozzo, W; Di Fiore, L; Di Lieto, A; Di Virgilio, A; Dietz, A; Drago, M; Endroczi, G; Fafone, V; Ferrante, I; Ferrini, F; Fidecaro, F; Fiori, I; Flaminio, R; Forte, La; Fournier, Jd; Franc, J; Franco, S; Frasca, S; Frasconi, F; Galimberti, M; Gammaitoni, L; Garufi, F; Gaspar, Me; Gemme, G; Genin, E; Gennai, A; Giazotto, A; Gouaty, R; Granata, M; Guidi, Gm; Heidmann, A; Heitmann, H; Hello, P; Hemming, G; Jaranowski, P; Jonker, Rjg; Kasprzack, M; Kowalska, I; Krolak, A; Leroy, N; Letendre, N; Li, Tgf; Lorenzini, M; Loriette, V; Losurdo, G; Majorana, E; Maksimovic, I; Malvezzi, V; Man, N; Mantovani, M; Marchesoni, F; Marion, F; Marque, J; Martelli, F; Masserot, A; Meidam, J; Michel, C; Milano, L; Minenkov, Y; Mohan, M; Morgado, N; Mosca, S; Mours, B; Naticchioni, L; Neri, I; Nocera, F; Palladino, L; Palomba, C; Paoletti, F; Paoletti, R; Parisi, M; Pasqualetti, A; Passaquieti, R; Passuello, D; Pichot, M; Piergiovanni, F; Pinard, L; Poggiani, R; Prodi, Ga; Punturo, M; Puppo, P; Rabeling, Ds; Racz, I; Rapagnani, P; Re, V; Regimbau, T; Ricci, F; Robinet, F; Rocchi, A; Rolland, L; Romano, R; Rosinska, D; Ruggi, P; Saracco, E; Sassolas, B; Sentenac, D; Sperandio, L; Sturani, R; Swinkels, B; Tacca, M; Taffarello, L; ter Braack, Apm; Toncelli, A; Tonelli, M; Torre, O; Tournefier, E; Travasso, F; Vajente, G; van den Brand, Jfj; Van den Broeck, C; van der Putten, S; Vasuth, M; Vavoulidis, M; Vedovato, G; Verkindt, D; Vetrano, F; Vicere, A; Vinet, Jy; Vitale, S; Vocca, H; Ward, Rl; Was, M; Yvert, M; Zadrozny, A; Zendri, Jp. - 467:(2013). (Intervento presentato al convegno 9TH LISA SYMPOSIUM tenutosi a Paris, FRANCE).
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1408646
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